{
  "id": "1508.03580",
  "version": "v1",
  "published": "2015-08-14T17:54:25.000Z",
  "updated": "2015-08-14T17:54:25.000Z",
  "title": "Impact of cosmological satellites on the vertical heating of the Milky Way disc",
  "authors": [
    "R. Moetazedian",
    "A. Just"
  ],
  "comment": "20 pages, 24 figures, 3 tables",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "We present a high resolution study of the impact of realistic satellite galaxies, extracted from cosmological simulations of Milky Way haloes including 6 Aquarius suites and Via Lactea \\rom{2}, on the dynamics of the galactic disc. The initial conditions for the multi-component Milky Way galaxy were generated using the GalIC code, to ensure a system in real equilibrium state prior to addition of satellites. The candidate subhaloes that came closer than 25 kpc to the centre of the host DM haloes, with initial mass $M_\\textrm{tid}$ $\\ge$ 10$^{8}$=0.003 $M_\\textrm{tid}$/$M_\\textrm{disc}$, were identified, inserted into our high resolution N-body simulations and evolved for 2 Gyrs. We quantified the vertical heating due to such impacts by measuring the disc thickness, root-mean-square of $z$-coordinate, and vertical velocity dispersion $\\sigma_{z}^{2}$ across the disc. According to our analysis the strength of the heating is strongly dependent on the high mass end of the subhalo distribution from the cosmological simulations. The mean increase of the vertical dispersion is $\\sim$ 25 km$^{2}$s$^{-2}$Gyr$^{-1}$ for R $>$ 4 kpc while, if we exclude Aq-F-2 results, the mean heating is $<$ 12 km$^{2}$s$^{-2}$Gyr$^{-1}$. The observed vertical heating rate in the solar neighbourhood has a value of 67 km$^{2}$s$^{-2}$Gyr$^{-1}$; taking into account the 1$\\sigma$ statistical dispersion around the mean we lie just below the observed value of 144 km$^{2}$s$^{-2}$ after 2 Gyrs. We observed a general flaring of the disc height in the case of all 7 simulations in the outer disc where the thickness was increased by $\\sim$ 40% at 15 kpc. The 1$\\sigma$ cosmic variance corresponds to doubling the disc thickness in the outer region.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-08-14T17:54:25.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "milky way disc",
      "vertical heating",
      "cosmological satellites",
      "disc thickness",
      "high resolution n-body simulations"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 20,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}